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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S235(2), p. 81-81, 2006

DOI: 10.1017/s1743921306005187

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The Distribution of Bar Strengths in Disk Galaxies

Journal article published in 2006 by R. Buta, E. Laurikainen, H. Salo, J. H. Knapen ORCID, D. L. Block
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractBars are the most important features that redistribute angular momentum and drive secular evolution in disk galaxies. We have derived the distribution of bar strengths in spirals and the Fourier properties of early-type galaxy bars in order to evaluate recent models of bar-halo angular momentum transfer and external gas accretion. A few results are presented here.

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